Velocities and the line-of-sight distribution of molecular clouds close to the Galactic centre

Details Velocities and the line-of-sight distribution of molecular clouds close to the Galactic centre Velocities and the line-of-sight distribution of molecular clouds close to the Galactic centre

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237p...7c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 7P-13P.

Astronomy and Astrophysics

Astronomy

2

Galactic Nuclei, Infrared Sources (Astronomy), Line Of Sight, Molecular Clouds, Velocity Distribution, Absorption Spectra, High Resolution, High Temperature Gases

Scientific paper

Blends among absorption profiles produced by molecular clouds detected in high-resolution spectra of bright infrared sources clustered around the direction of the Galactic center are reexamined. It is concluded, in agreement with earlier kinematic studies of hot neutral gas in the circumnuclear ring, that the Galactic center and the local standard of rest are separating at about 40 km/s.

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